CWWDL 14646

0.00 UTI

0.33

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AA

Number of members (P>50%) 33

Radius (P>50% members) 12.1 [arcmin]

C_N 0.33 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWWDL 14646 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry, and a small percentage with at least one entry reported in the same catalogue. See table with shared members information.

Near-solar metallicity Very young

Data

🔍 Search references for CWWDL 14646 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	279.446	-0.344	2.135	2.755	-8.433	0.178
Chi et al.	2023	279.447	-0.305	2.146	2.75	-8.395	9.447

💡 Note: The UCC values are estimated from its identified members.

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	Bfr	BSS
Chi et al.	2023	–	–	–	6	0.200	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UPK 41	100.0	279.58	0.42	2.09	2.63	-8.29	-5.04	0.69
OC 0059	72.7	279.46	-0.37	2.14	2.83	-8.45	2.52	0.0
OC 0062	21.2	279.39	0.44	2.06	2.55	-8.24	1.1	0.0
CWWDL 14647	18.2	279.98	0.64	2.09	2.52	-8.25	-7.7	0.0

💡 Note: The % column shows the percentage of members that CWWDL 14646 shares with each listed object.

Visualization

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